Near infrared reflection spectra of ammonia frost: Interpretation of the upper clouds of Saturn
- 30 November 1978
- journal article
- Published by Elsevier in Journal of Quantitative Spectroscopy and Radiative Transfer
- Vol. 20 (5) , 481-490
- https://doi.org/10.1016/0022-4073(78)90052-3
Abstract
No abstract availableThis publication has 17 references indexed in Scilit:
- A model for the temperature inversion within the atmosphere of SaturnIcarus, 1977
- The abundances of ammonia in the atmospheres of Jupiter, Saturn, and TitanIcarus, 1977
- Jupiter: An inhomogeneous atmospheric model analysis of spatial variations of the H2 4-0 S(1) lineIcarus, 1977
- The atmosphere of Saturn: An infrared perspectiveIcarus, 1977
- The influence of ethane and acetylene upon the thermal structure of the Jovian atmosphereIcarus, 1975
- Optical constants of solid ammonia in the infrared*Journal of the Optical Society of America, 1975
- The 7.5- to 13.5-MICRON Spectrum of SaturnThe Astrophysical Journal, 1974
- Preliminary Data on the Optical Properties of Solid Ammonia and Scattering Parameters for Ammonia Cloud ParticlesJournal of the Atmospheric Sciences, 1973
- The Infrared Spectra of Jupiter and Saturn at 1.2-4.2 MicronsThe Astrophysical Journal, 1970
- Model atmospheres of the major planetsThe Astrophysical Journal, 1967